The position and magnitude of 1449 stars listed in "Seoung Kyung" (by Byung Kil Nahm, 1861) are compared with those in modern western star catalogues for their identification. 923 stars out of 1449 stars were identified within the range of accuracy. Δ α ≤ 20 s .0 , Δ δ ≤ 1 ′ .0 a n d Δ m = 0 o r ± 1 . When Δ α a n d Δ δ increased to Δ α ≤ 1 m . 0 , Δ δ ≤ 15 ′ .0 a n d Δ m = 0 or +1, 399 more stars could be included in the list.

Abstract
1. 序論
2. 星鏡의 內容
3. 별의 同定方法
4. 同定의 結果
參考文獻
附錄

• 韓郁(Department of Earth Science, Korea Military Academy) | Wook Hahn
• 兪景老(Department of Earth Science, College of Education, Seoul National University) | Kyung Loh Yu